NGC 4065:修订间差异
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| work=Results for NGC 4065 |
| work=Results for NGC 4065 |
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| url=http://nedwww.ipac.caltech.edu/ |
| url=http://nedwww.ipac.caltech.edu/ |
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| access-date=2019-02-01 |
| access-date=2019-02-01 |
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| archive-date=2008-12-16 |
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| archive-url=https://web.archive.org/web/20081216032441/http://nedwww.ipac.caltech.edu/ |
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| dead-url=no |
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| ra = {{RA|12|04|06.2}}<ref name="ned" /> |
| ra = {{RA|12|04|06.2}}<ref name="ned" /> |
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| dec = {{DEC|20|14|06}}<ref name="ned" /> |
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'''NGC 4065'''是一个位于[[后发座]]的[[椭圆星系]],距离地球3亿光年<ref>{{Cite web|url=https://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+4065&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES|title=Your NED Search Results|website=ned.ipac.caltech.edu|access-date=2019-02-02}}</ref><ref>{{Cite web|url=http://spider.seds.org/ngc/revngcic.cgi?NGC4065|title=Revised NGC Data for NGC 4065|website=spider.seds.org|access-date=2019-02-02}}</ref>。NGC 4065于1785年4月27日由[[威廉·赫歇爾]]首次发现,1832年4月29日由[[約翰·赫歇爾]]再次发现,并被列为'''NGC 4057'''<ref>{{Cite web|url=https://cseligman.com/text/atlas/ngc40a.htm#4065|title=New General Catalog Objects: NGC 4050 - 4099|website=cseligman.com|access-date=2019-01-15}}</ref>。NGC 4065属于{{tsl|en|NGC 4065 Group|NGC 4065星系团}}<ref name=":7" /><ref name=":3">{{Cite journal|last1=Doe|first1=Stephen M.|last2=Ledlow|first2=Michael J.|last3=Burns|first3=Jack O.|last4=White|first4=Richard A.|date=1995-07-01|title=ROSAT Observations of Five Poor Galaxy Clusters with Extended Radio Sources|journal=The Astronomical Journal|volume=110|pages=46|doi=10.1086/117496|issn=0004-6256|bibcode=1995AJ....110...46D}}</ref><ref name=":5">{{Cite journal|last1=Freeland|first1=E.|last2=Stilp|first2=A.|last3=Wilcots|first3=E.|date=2009-07-01|title=H I Observations of Five Groups of Galaxies|journal=The Astronomical Journal|volume=138|issue=1|pages=295–304|doi=10.1088/0004-6256/138/1/295|issn=0004-6256|bibcode=2009AJ....138..295F|arxiv=0905.3907|s2cid=15714969}}</ref>,与[[NGC 4061]]组成一对[[交互作用星系]]<ref name=":4">{{Cite journal|last1=Batuski|first1=David J.|last2=Hanisch|first2=Robert J.|last3=Burns|first3=Jack O.|date=1992-04-01|title=VLA observations of radio sources in interacting galaxy pairs in poor clusters|journal=The Astronomical Journal|volume=103|pages=1077–1083|doi=10.1086/116126|issn=0004-6256|bibcode=1992AJ....103.1077B}}</ref><ref name=":7">{{Cite journal|last1=Venkatesan|first1=T. C. A.|last2=Batuski|first2=David J.|last3=Hanisch|first3=Robert J.|last4=Burns|first4=Jack O.|date=November 20, 1994|title=Why do head-tail sources exist in poor clusters of galaxies?|url=https://archive.org/details/sim_astrophysical-journal_1994-11-20_436_1/page/67|journal=The Astrophysical Journal|language=en|volume=436|pages=67–78|doi=10.1086/174881|issn=0004-637X|bibcode=1994ApJ...436...67V}}</ref>。 |
'''NGC 4065'''是一个位于[[后发座]]的[[椭圆星系]],距离地球3亿光年<ref>{{Cite web|url=https://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+4065&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES|title=Your NED Search Results|website=ned.ipac.caltech.edu|access-date=2019-02-02|archive-date=2022-06-29|archive-url=https://web.archive.org/web/20220629033734/https://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+4065&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES|dead-url=no}}</ref><ref>{{Cite web|url=http://spider.seds.org/ngc/revngcic.cgi?NGC4065|title=Revised NGC Data for NGC 4065|website=spider.seds.org|access-date=2019-02-02|archive-date=2019-02-03|archive-url=https://web.archive.org/web/20190203030655/http://spider.seds.org/ngc/revngcic.cgi?NGC4065|dead-url=no}}</ref>。NGC 4065于1785年4月27日由[[威廉·赫歇爾]]首次发现,1832年4月29日由[[約翰·赫歇爾]]再次发现,并被列为'''NGC 4057'''<ref>{{Cite web|url=https://cseligman.com/text/atlas/ngc40a.htm#4065|title=New General Catalog Objects: NGC 4050 - 4099|website=cseligman.com|access-date=2019-01-15|archive-date=2022-06-30|archive-url=https://web.archive.org/web/20220630065001/https://cseligman.com/text/atlas/ngc40a.htm#4065|dead-url=no}}</ref>。NGC 4065属于{{tsl|en|NGC 4065 Group|NGC 4065星系团}}<ref name=":7" /><ref name=":3">{{Cite journal|last1=Doe|first1=Stephen M.|last2=Ledlow|first2=Michael J.|last3=Burns|first3=Jack O.|last4=White|first4=Richard A.|date=1995-07-01|title=ROSAT Observations of Five Poor Galaxy Clusters with Extended Radio Sources|journal=The Astronomical Journal|volume=110|pages=46|doi=10.1086/117496|issn=0004-6256|bibcode=1995AJ....110...46D}}</ref><ref name=":5">{{Cite journal|last1=Freeland|first1=E.|last2=Stilp|first2=A.|last3=Wilcots|first3=E.|date=2009-07-01|title=H I Observations of Five Groups of Galaxies|journal=The Astronomical Journal|volume=138|issue=1|pages=295–304|doi=10.1088/0004-6256/138/1/295|issn=0004-6256|bibcode=2009AJ....138..295F|arxiv=0905.3907|s2cid=15714969}}</ref>,与[[NGC 4061]]组成一对[[交互作用星系]]<ref name=":4">{{Cite journal|last1=Batuski|first1=David J.|last2=Hanisch|first2=Robert J.|last3=Burns|first3=Jack O.|date=1992-04-01|title=VLA observations of radio sources in interacting galaxy pairs in poor clusters|journal=The Astronomical Journal|volume=103|pages=1077–1083|doi=10.1086/116126|issn=0004-6256|bibcode=1992AJ....103.1077B}}</ref><ref name=":7">{{Cite journal|last1=Venkatesan|first1=T. C. A.|last2=Batuski|first2=David J.|last3=Hanisch|first3=Robert J.|last4=Burns|first4=Jack O.|date=November 20, 1994|title=Why do head-tail sources exist in poor clusters of galaxies?|url=https://archive.org/details/sim_astrophysical-journal_1994-11-20_436_1/page/67|journal=The Astrophysical Journal|language=en|volume=436|pages=67–78|doi=10.1086/174881|issn=0004-637X|bibcode=1994ApJ...436...67V}}</ref>。 |
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==参考== |
==参考== |
2022年9月9日 (五) 06:29的最新版本
NGC 4065 | |
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观测资料(J2000 曆元) | |
星座 | 后发座 |
赤经 | 12h 04m 06.2s[1] |
赤纬 | 20° 14′ 06″[1] |
紅移 | 0.021101[1] |
徑向速度 | 6326 km/s[1] |
距离 | 300 Mly(91 Mpc)[1] |
属于 | NGC 4065星系群 |
视星等 (V) | 13.58[1] |
特征 | |
类型 | E[1] |
大小 | ~120,000 ly(37 kpc)[1] |
角直徑 (V) | 1.1 x 1.0[1] |
其他名称 | |
NGC 4057, MCG +04-29-007, PGC 038156, UGC 07050, VV 179a[1] | |
NGC 4065是一个位于后发座的椭圆星系,距离地球3亿光年[2][3]。NGC 4065于1785年4月27日由威廉·赫歇爾首次发现,1832年4月29日由約翰·赫歇爾再次发现,并被列为NGC 4057[4]。NGC 4065属于NGC 4065星系团[5][6][7],与NGC 4061组成一对交互作用星系[8][5]。
参考
[编辑]- ^ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 NASA/IPAC Extragalactic Database. Results for NGC 4065. [2019-02-01]. (原始内容存档于2008-12-16).
- ^ Your NED Search Results. ned.ipac.caltech.edu. [2019-02-02]. (原始内容存档于2022-06-29).
- ^ Revised NGC Data for NGC 4065. spider.seds.org. [2019-02-02]. (原始内容存档于2019-02-03).
- ^ New General Catalog Objects: NGC 4050 - 4099. cseligman.com. [2019-01-15]. (原始内容存档于2022-06-30).
- ^ 5.0 5.1 Venkatesan, T. C. A.; Batuski, David J.; Hanisch, Robert J.; Burns, Jack O. Why do head-tail sources exist in poor clusters of galaxies?. The Astrophysical Journal. November 20, 1994, 436: 67–78. Bibcode:1994ApJ...436...67V. ISSN 0004-637X. doi:10.1086/174881 (英语).
- ^ Doe, Stephen M.; Ledlow, Michael J.; Burns, Jack O.; White, Richard A. ROSAT Observations of Five Poor Galaxy Clusters with Extended Radio Sources. The Astronomical Journal. 1995-07-01, 110: 46. Bibcode:1995AJ....110...46D. ISSN 0004-6256. doi:10.1086/117496.
- ^ Freeland, E.; Stilp, A.; Wilcots, E. H I Observations of Five Groups of Galaxies. The Astronomical Journal. 2009-07-01, 138 (1): 295–304. Bibcode:2009AJ....138..295F. ISSN 0004-6256. S2CID 15714969. arXiv:0905.3907 . doi:10.1088/0004-6256/138/1/295.
- ^ Batuski, David J.; Hanisch, Robert J.; Burns, Jack O. VLA observations of radio sources in interacting galaxy pairs in poor clusters. The Astronomical Journal. 1992-04-01, 103: 1077–1083. Bibcode:1992AJ....103.1077B. ISSN 0004-6256. doi:10.1086/116126.
外部链接
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